Four Lectures on Relativity and Space Formula Map
Formula Map
Section titled “Formula Map”Review layer: these are OCR/PDF-text formula candidates. Promote only after scan verification, mathematical transcription, and notation review.
170
Formula and equation candidates.
57
Strong formula candidates.
34
Reviewable relation candidates.
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Formula Families
Section titled “Formula Families”| Family | Candidates |
|---|---|
| General Equation Candidates | 148 |
| Waves, Lines, Radiation, And Frequency | 14 |
| Symbolic AC And Complex Quantities | 5 |
| Power, Energy, Work, And Efficiency | 3 |
Highest-Priority Candidates
Section titled “Highest-Priority Candidates”| Candidate | Family | OCR/PDF text | Routes |
|---|---|---|---|
four-lectures-relativity-space-eq-candidate-0073strong-formula-candidate | symbolic-ac | at A and is tan C02 = Vijv^ (thus being greater) when the | source workbench |
four-lectures-relativity-space-eq-candidate-0126strong-formula-candidate | symbolic-ac | R = j/VK. (15) | source workbench |
four-lectures-relativity-space-eq-candidate-0045strong-formula-candidate | general-equation-candidates | If then vx = 0.9c and V2 = 0.9c, v = 1.8c/1.81 = 0.9945c; | source workbench |
four-lectures-relativity-space-eq-candidate-0141strong-formula-candidate | symbolic-ac | C = 2t sin r, | source workbench |
four-lectures-relativity-space-eq-candidate-0004strong-formula-candidate | general-equation-candidates | c = ~7E=^ = 3 X IQio cm., | source workbench |
four-lectures-relativity-space-eq-candidate-0006strong-formula-candidate | general-equation-candidates | value - that is, assume x = 0, t = 0, x’ = 0, t’ = 0, | source workbench |
four-lectures-relativity-space-eq-candidate-0007strong-formula-candidate | waves-radiation | 1. Since x’i’ has relative to xi the velocity f, it is, for a;’ = 0:ax - bt = 0, | source workbench |
four-lectures-relativity-space-eq-candidate-0011strong-formula-candidate | general-equation-candidates | x’ = a{x - vt) 1 | source workbench |
four-lectures-relativity-space-eq-candidate-0013strong-formula-candidate | general-equation-candidates | i’ = ^= or i = ^= (2) | source workbench |
four-lectures-relativity-space-eq-candidate-0015strong-formula-candidate | general-equation-candidates | from the train^ - is U = X2’ - Xi ; in track coordinates - | source workbench |
four-lectures-relativity-space-eq-candidate-0017strong-formula-candidate | general-equation-candidates | between the same events is T = to - ti. However, by (2) : | source workbench |
four-lectures-relativity-space-eq-candidate-0020strong-formula-candidate | general-equation-candidates | the time i\\ that is, the length of the train is L = X\- X2. | source workbench |
four-lectures-relativity-space-eq-candidate-0023strong-formula-candidate | general-equation-candidates | s^ = (X2 - x^y + {u -hy = (xo’ - xi’Y + {k - uY =s’^ | source workbench |
four-lectures-relativity-space-eq-candidate-0024strong-formula-candidate | general-equation-candidates | {X2 - xi)2 - c\U -hy = (x./ - Xi’Y - c\t,’ - h’Y, (5) | source workbench |
four-lectures-relativity-space-eq-candidate-0026strong-formula-candidate | general-equation-candidates | w = ct (6) | source workbench |
four-lectures-relativity-space-eq-candidate-0028strong-formula-candidate | general-equation-candidates | *S^ = (0:2 - Xi)^ - {w-i - WiY = | source workbench |
four-lectures-relativity-space-eq-candidate-0030strong-formula-candidate | general-equation-candidates | u = jet’, (10) | source workbench |
four-lectures-relativity-space-eq-candidate-0031strong-formula-candidate | general-equation-candidates | x’ = -r==l or: X = ~. (11) | source workbench |
four-lectures-relativity-space-eq-candidate-0033strong-formula-candidate | general-equation-candidates | S’- = (x, - x,y + (i/2 - yiY + (22 - z,y + {U2 - u^y = | source workbench |
four-lectures-relativity-space-eq-candidate-0036strong-formula-candidate | general-equation-candidates | light- by (3) and (4), L = 0 and T = oo. That is, on | source workbench |
four-lectures-relativity-space-eq-candidate-0039strong-formula-candidate | waves-radiation | be V = Vi -{- V2 = 1.8c, or greater than the velocity of | source workbench |
four-lectures-relativity-space-eq-candidate-0043strong-formula-candidate | waves-radiation | velocity V2, it is Xi = v^h, and substituting this in the | source workbench |
four-lectures-relativity-space-eq-candidate-0050strong-formula-candidate | power-energy | The kinetic energy of 1 kg. weight of matter, Eq = mc^, | source workbench |
four-lectures-relativity-space-eq-candidate-0052strong-formula-candidate | general-equation-candidates | F = HP (1) | source workbench |
four-lectures-relativity-space-eq-candidate-0053strong-formula-candidate | general-equation-candidates | F=KQ, (2) | source workbench |
four-lectures-relativity-space-eq-candidate-0054strong-formula-candidate | general-equation-candidates | F = gN, (3) | source workbench |
four-lectures-relativity-space-eq-candidate-0055strong-formula-candidate | general-equation-candidates | F = CR, (4) | source workbench |
four-lectures-relativity-space-eq-candidate-0056strong-formula-candidate | general-equation-candidates | W = Mvy2, (5) | source workbench |
four-lectures-relativity-space-eq-candidate-0057strong-formula-candidate | general-equation-candidates | a = F/M, (6) | source workbench |
four-lectures-relativity-space-eq-candidate-0063strong-formula-candidate | general-equation-candidates | per cent, and the acceleration thus is a = 0.1^ = 2.2 miles | source workbench |